V. Gonzalez-Perez
Do model emission line galaxies live in filaments at z∼1?
Gonzalez-Perez, V.; Cui, W.; Contreras, S.; Baugh, C.M.; Comparat, J.; Griffin, A.J.; Helly, J.; Knebe, A.; Lacey, C.; Norberg, P.
Authors
W. Cui
S. Contreras
Professor Carlton Baugh c.m.baugh@durham.ac.uk
Professor
J. Comparat
A.J. Griffin
Dr John Helly j.c.helly@durham.ac.uk
Chief Experimental Officer
A. Knebe
Professor Cedric Lacey cedric.lacey@durham.ac.uk
Emeritus Professor
Professor Peder Norberg peder.norberg@durham.ac.uk
Professor
Abstract
Current and future cosmological surveys are targeting star-forming galaxies at z∼ 1 with nebular emission lines. We use a state-of-the-art semi-analytical model of galaxy formation and evolution to explore the large scale environment of star-forming emission line galaxies (ELGs). Model ELGs are selected such that they can be compared directly with the DEEP2, VVDS, eBOSS-SGC and DESI surveys. The large scale environment of the ELGs is classified using velocity-shear-tensor and tidal-tensor algorithms. Half of the model ELGs live in filaments and about a third in sheets. Model ELGs which reside in knots have the largest satellite fractions. We find that the shape of the mean halo occupation distribution of model ELGs varies widely for different large scale environments. To interpret our results, we also study fixed number density samples of ELGs and galaxies selected using simpler criteria, with single cuts in stellar mass, star formation rate and [OII] luminosity. The fixed number density ELG selection produces samples that are close to L[OII] and SFR selected samples for densities above 10−4.2h3Mpc−3. ELGs with an extra cut in stellar mass applied to fix their number density, present differences in sheets and knots with respect to the other samples. ELGs, SFR and L[OII] selected samples with equal number density have similar large scale bias but their clustering below separations of 1h−1Mpc is different.
Citation
Gonzalez-Perez, V., Cui, W., Contreras, S., Baugh, C., Comparat, J., Griffin, A., Helly, J., Knebe, A., Lacey, C., & Norberg, P. (2020). Do model emission line galaxies live in filaments at z∼1?. Monthly Notices of the Royal Astronomical Society, 498(2), 1852-1870. https://doi.org/10.1093/mnras/staa2504
Journal Article Type | Article |
---|---|
Acceptance Date | Aug 12, 2020 |
Online Publication Date | Aug 20, 2020 |
Publication Date | 2020-10 |
Deposit Date | Aug 21, 2020 |
Publicly Available Date | Sep 18, 2020 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 498 |
Issue | 2 |
Pages | 1852-1870 |
DOI | https://doi.org/10.1093/mnras/staa2504 |
Public URL | https://durham-repository.worktribe.com/output/1263689 |
Files
Published Journal Article
(5.6 Mb)
PDF
Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
You might also like
The two-point correlation function covariance with fewer mocks
(2023)
Journal Article
The DESI Bright Galaxy Survey: Final Target Selection, Design, and Validation
(2023)
Journal Article
A sparse regression approach for populating dark matter haloes and subhaloes with galaxies
(2022)
Journal Article
Solving small-scale clustering problems in approximate light-cone mocks
(2022)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search